Group Structure of Einstein Equations: Casimir Operator & Conserved Quantities

In summary: The metric can also be written asg_{ab}=\sum_{i,j}g_{ij}which is a four-metric.The canonical momentum is given by\pi_{ab}=\frac{\partial \mathcal{L}}{\partial g_{ab}}which is correct. In GR or its quantum version physicists asume that metric can be written by means of a foliation. g_{ab}=dt^{2}+g_{ij}dx^{i}dx^{j} hence i and j runs only over space variables...The canonical momentum is given by\pi_{ab}=\frac{\partial \
  • #1
Klaus_Hoffmann
86
1
if we consider the Group structure of [tex] [ \pi _{ij} , g_{ab}]= \delta _{ia,jb} [/tex]

of the Einstein equation for the momenta and metric, could we obtain its Casimir Operator, conserved quantities and so on?
 
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  • #2
It may be a misunderstanding on my part, by the expression you've given above makes no sense. Care to give us some context?
 
  • #3
Yes of course , if you have the Einstein Lagrangian [tex] \sqrt{-g}R [/tex]

then the Einstein Group (as my definition) would be the group that leaves the Lagrangian invariant so if you change the metric in the from [tex] Fg_{ab} \rightarrow h_{ab} [/tex] where h and g are the transformed metric under the group G so the Lagrangian remains the same but a surface term, so using NOether's theorem the infinitesimal generators of the Group will be the (physical) conserved quantities.
 
  • #4
I shoehorn may be referring to the [tex]\left[\;\;,\;\;\right][/tex] symbol. What do you mean by that?
 
  • #5
The [ , ] symbol is most likely a commutator (see for instance Wald, GR, pg 18). Given two smooth vector fields v and w, a commutator defines a new vector field:

[v,w](f) = v(w(f)) - w(v(f))

Of course in this case v and w are rank 2 tensor fields, not vector fields. I believe it's sensible to talk about the commutator of a rank 2 tensor field, but I'd have to look up the details.

I would furthermore assume that the [itex]\pi[/itex] are cannonical momenta in the Hamiltonian formulation of GR.

Unfortunately I don't know the answer to the original poster's questions offhand - I was hoping that someone else would tackle it.
 
  • #6
I'm mystified. The OP seems to be defining an algebra using a three-momentum ([itex]\pi^{ij}[/itex]) and a four-metric ([itex]g_{ab}[/itex]). This is obviously fruitless since, without further restrictive qualification, such an algebra can't even be defined.

What's even more confusing is that he's mixing in the Einstein-Hilbert Lagrangian with manifestly three-dimensional quantities such as the three-momentum.
 
  • #7
shoehorn said:
I'm mystified. The OP seems to be defining an algebra using a three-momentum ([itex]\pi^{ij}[/itex]) and a four-metric ([itex]g_{ab}[/itex]). This is obviously fruitless since, without further restrictive qualification, such an algebra can't even be defined.

What's even more confusing is that he's mixing in the Einstein-Hilbert Lagrangian with manifestly three-dimensional quantities such as the three-momentum.


Maybe he meant the metric induced on 3-d space, but I usually see that written as [itex]\Sigma_{ij}[/itex].
 
  • #8
pervect said:
Maybe he meant the metric induced on 3-d space, but I usually see that written as [itex]\Sigma_{ij}[/itex].

Care to give me a link to where the three-metric is denoted by a capital sigma? In the literate it is almost always either g or lower case gamma. Regardless, even if he was talking about the three-metric, his expression still doesn't make any sense since any conceivable algebra would have to respect the symmetry of the three-metric and its momentum. If you look at the expression the OP gave, the rhs isn't symmetric in (i,j) or (a,b).

What's more, he should have some form of distribution on the rhs also.
 
  • #9
shoehorn said:
Care to give me a link to where the three-metric is denoted by a capital sigma?

I thought Wald did, but I see now that I was confused, [itex]\Sigma_t[/itex] is a spacelike slice at time t, not a metric.

<snip some silly stuff I wrote earlier>

So I have to agree it's not really clear what the original question is about, but it seems to me that we can be polite about asking the OP what he had in mind.

BTW, I'm not really confident that [] represents commutators, maybe they're Poisson brackets.
 
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  • #10
Surely

[tex]\pi_{ab} = \frac{\partial \mathcal{L}}{\partial g_{ab}}[/tex]

which is not three-momenta, but instead the canonical momenta, given that [itex]g_{ab}[/itex] is the field variable.
 
  • #11
masudr said:
Surely

[tex]\pi_{ab} = \frac{\partial \mathcal{L}}{\partial g_{ab}}[/tex]

which is not three-momenta, but instead the canonical momenta, given that [itex]g_{ab}[/itex] is the field variable.

When I say "three-momenta" I'm taking it as given that I'm referring to "field momentum canonically conjugate to the three-metric on a spatial slice".
 
  • #12
shoehorn said:
When I say "three-momenta" I'm taking it as given that I'm referring to "field momentum canonically conjugate to the three-metric on a spatial slice".

Ah, my mistake. My ignorance has been publically displayed.
 
  • #13
masudr said:
Ah, my mistake. My ignorance has been publically displayed.

Let me clarify it even further for you. When I say "three-momentum" I use it in exactly the same sense that almost every paper I've ever seen on canonical general relativity uses.

Also, your definition of the canonical momentum

[tex]\pi_{ab}= \frac{\partial\mathcal{L}}{\partial g_{ab}}[/tex]

is incorrect for several reasons.
 
  • #14
in GR or its quantum version physicist asume that metric can be written by means of a foliation.

[tex] g_{ab}=dt^{2}+g_{ij}dx^{i}dx^{j} [/tex] hence i and j runs only over space variables x,y,z
 
  • #15
masudr said:
Surely

[tex]\pi_{ab} = \frac{\partial \mathcal{L}}{\partial g_{ab}}[/tex]

which is not three-momenta, but instead the canonical momenta, given that [itex]g_{ab}[/itex] is the field variable.

I've seen [tex]\frac{\pi^{ij}}{16 \pi} = \pi_{\mathrm{true}}^{ij} = \frac{\delta L}{\delta g_{ij}}[/tex]

for instance, MTW pg 521

so you're very close, but apparently you won't be getting any cigar from shoehorn :-). This assumes [itex]g_{ij}[/itex] is a three metric, in the sense that's already been discussed. The difference betweeen [itex]\partial[/itex] and [itex]\delta[/itex] is the difference between the partial derivative of a function and a functional derivative (the action is a functional, i.e. it's a map from a function to a scalar).

I hope this is both more helpful than shoehorn's terse reply and also close to being correct (the textbook quote is definitely quoted correctly) unfortunately I don't really work much with the ADM formalism of which this is a part.

If you have Goldstein, Classical Mechanics, you might also look at the section on pg 420 about the symmetry groups of mechanical systems - rereading this makes it seem pretty likely to me that the [ ] are indeed Poisson brackets, though I can't quite justify the specific relation in the original question in my mind.
 
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  • #16
Please don't take my abrupt comments as being rude; I certainly don't intend to be so and if I've come across that way, my apologies.

You claim that MTW say that the momentum is defined by:

[tex]\pi^{ij} = \frac{\delta L}{\delta g_{ij}}[/tex]

You're correct when you claim that MTW say this is how the momentum is defined. However, the important point is that MTW are wrong! This is not as heretical as it may sound. Consider, for example, an ordinary classical system with generalised coordinates [itex]q^i[/tex], generalised velocities [itex]\dot{q}^i[/itex], and a Lagrangian [itex]L[/itex]. In this trivial case we don't define the momentum conjugate to [itex]q^i[/itex] as

[tex]\pi_i = \frac{\partial L}{\partial q^i}[/tex]

This is the analogue of what you've written for the momentum in general relativity. The correct way to define the momentum is of course

[tex]\pi_i = \frac{\partial L}{\partial\dot{q}^i}[/tex]

This is a trivial observation. The correct way to define the three-momentum in general relativity is then

[tex]\pi^{ij} = \frac{\delta \mathcal{L}}{\delta\dot{g}_{ij}}[/tex]

where the Lagrangian density (and note that the correct thing to use is the Lagrangian density, not the Lagrangian itself due to the possible presence of surface terms) is understood to have been expressed in terms of the first and second fundamental forms of a hypersurface in the spacetime.

If you work through the calculations you'll find that my correct way of defining the three-momentum gives

[tex]\pi^{ij} = \sqrt{g}(g^{ij}K - K^{ij})[/tex]

On the other hand, if you use MTW's incorrect definition, you'll get something a whole lot more complicated (you'll get the euler-lagrange equations actually, as you could have noticed had you thought a little bit about the equation in MTW before transcribing it).
 
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  • #17
General cigar shortage, it appears (:
 
  • #18
masudr said:
General cigar shortage, it appears (:

LOL, yep, but educational.
 

Related to Group Structure of Einstein Equations: Casimir Operator & Conserved Quantities

1. What is the significance of the Casimir Operator in the group structure of Einstein equations?

The Casimir Operator is a mathematical operator that plays a crucial role in the group structure of Einstein equations. It is used to generate the symmetries of the equations, which are essential for understanding the underlying physical principles.

2. How does the Casimir Operator relate to conserved quantities in Einstein equations?

The Casimir Operator is directly related to the conserved quantities in Einstein equations. It generates these quantities through the symmetries it generates, providing a powerful tool for understanding the conservation laws in the equations.

3. Can the Casimir Operator be used to simplify the group structure of Einstein equations?

Yes, the Casimir Operator can be used to simplify the group structure of Einstein equations. It allows for the identification of subgroups within the larger group structure, making it easier to understand and analyze the equations.

4. Are there any practical applications of understanding the group structure of Einstein equations?

Yes, understanding the group structure of Einstein equations has practical applications in various fields, such as cosmology and general relativity. It allows for a deeper understanding of the underlying principles and can lead to new insights and discoveries.

5. How does the group structure of Einstein equations relate to other areas of physics?

The group structure of Einstein equations is closely related to other areas of physics, such as quantum mechanics and particle physics. It provides a framework for understanding the fundamental principles of these fields and how they relate to each other.

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